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Table 1.
Continuum ALMA observations.
Central wavelength | Time on-source | Cont. depth | Native beam | MRS | ALMA Band | Project code |
---|---|---|---|---|---|---|
[μm] | [min] | [mJy beam−1] | [″] | [″] | ||
(1) | (2) | (3) | (4) | (5) | (6) | (7) |
63 | 30 | 1.15 | 0.39 × 0.32 | 2.9 | 10 | 2017.1.00899.S |
88 | 172 | 1.36 | 0.36 × 0.31 | 3.4 | 9 | 2021.1.00726.S |
123 | 30 | 0.30 | 0.53 × 0.38 | 3.5 | 8 | 2016.1.00668.S |
149 | 124 | 0.040 | 0.44 × 0.35 | 4.5 | 7 | 2017.1.00899.S |
155 | 380 | 0.044 | 0.36 × 0.30 | 4.4 | 7 | 2018.1.00333.S |
211 | 148 | 0.017 | 0.54 × 0.46 | 5.1 | 6 | 2015.1.00883.S |
357 | 293 | 0.007 | 0.50 × 0.39 | 6.1 | 4 | 2019.1.00219.S |
572 | 31 | 0.019 | 0.35 × 0.30 | 4.0 | 3 | 2018.1.00119.S |
Notes. (1) Central rest-frame wavelength; (2) Integration time on-source; (3) Root mean square of the collapsed dataset; (4) Average size (FWHM) of the native beam, without uv-tapering; (5) Maximum recoverable scale; (6) ALMA receiver band; (7) ALMA project code.
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